James Webb Space Telescope Feed Post

Harvard ADS: Polycyclic aromatic hydrocarbon (PAH) luminous galaxies in JWST CEERS data

Paper abstract: It has been an unanswered question how many dusty galaxies have been undetected from the state-of-the-art observational surveys. JWST enables us to detect faint IR galaxies that have prominent polycyclic aromatic hydrocarbon (PAH) features in the mid-IR wavelengths. PAH is a valuable tracer of star formation and dust properties in the mid-infrared wavelength. The JWST Cosmic Evolution Early Release Science (CEERS) fields provide us with wavelength coverage from 7.7 to 21 \mum using six photometric bands of the mid-infrared instrument (MIRI). We have identified galaxies dominated by mid-IR emission from PAHs, termed PAH galaxies. From our multi-band photometry catalogue, we selected ten PAH galaxies displaying high flux ratios of \log(S_{15}/S_{10}) > 0.8. The SED fitting analysis indicates that these galaxies are star-forming galaxies with total IR luminosities of 10^{10} ~ 10^{11.5} L_{\odot} at z ~ 1. The morphology of PAH galaxies does not show any clear signatures of major merging or interaction within the MIRI resolution. The majority of them are on the star-formation main sequence at z ~ 1. Our result demonstrates that JWST can detect PAH emissions from normal star-forming galaxies at z ~ 1, in addition to ultra-luminous infrared galaxies (ULIRGs) or luminous infrared galaxies (LIRGs).